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Stability of Standing Accretion Shocks, With an Eye Toward Core Collapse Supernovae by John M. Blondin and others (2003)

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arxiv.org/abs/astro-ph/0210634
Primary standing-shock instability calculations, Astrophysical Journal 584, 971–980. The abstract contrasts radial stability with nonradial growth and vorticity generation at distorted shocks.

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  • Past exam of the astrophysics course of the University of Oxford / 2018 / 6 / a / Solution

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